1230908
doi
10.1126/science.1178312
oai:zenodo.org:1230908
Koch, D.
Jenkins, J.
Sasselov, D.
Gilliland, R.
Batalha, N.
Latham, D. W.
Caldwell, D.
Basri, G.
Brown, T.
Christensen-Dalsgaard, J.
Cochran, W. D.
DeVore, E.
Dunham, E.
Dupree, A. K.
Gautier, T.
Geary, J.
Gould, A.
Howell, S.
Kjeldsen, H.
Lissauer, J.
Marcy, G.
Meibom, S.
Morrison, D.
Tarter, J.
Kepler's Optical Phase Curve of the Exoplanet HAT-P-7b
Borucki, W. J.
info:eu-repo/semantics/openAccess
Creative Commons Zero v1.0 Universal
https://creativecommons.org/publicdomain/zero/1.0/legalcode
Ten days of photometric data were obtained during the commissioning phase of the Kepler mission, including data for the previously known giant transiting exoplanet HAT-P-7b. The data for HAT-P-7b show a smooth rise and fall of light from the planet as it orbits its star, punctuated by a drop of 130 ± 11 parts per million in flux when the planet passes behind its star. We interpret this as the phase variation of the dayside thermal emission plus reflected light from the planet as it orbits its star and is occulted. The depth of the occultation is similar in photometric precision to the detection of a transiting Earth-size planet for which the mission was designed.
Zenodo
2009-08-06
info:eu-repo/semantics/article
1230907
1579541677.664659
173556
md5:68ecca4d02d5549ae5ca26e598bdabfb
https://zenodo.org/records/1230908/files/article.pdf
public